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Scattering of Spinning Black Holes from Exponentiated Soft Factors

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Vines,  Justin
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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1812.06895.pdf
(プレプリント), 688KB

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引用

Guevara, A., Ochirov, A., & Vines, J. (2019). Scattering of Spinning Black Holes from Exponentiated Soft Factors. Journal of High Energy Physics, 2019(9):. doi:10.1007/JHEP09(2019)056.


引用: https://hdl.handle.net/21.11116/0000-0002-BB91-7
要旨
We provide evidence that the classical scattering of two spinning black holes
is controlled by the soft expansion of exchanged gravitons. We show how an
exponentiation of Cachazo-Strominger soft factors, acting on massive
higher-spin amplitudes, can be used to find spin contributions to the
aligned-spin scattering angle through one-loop order. The extraction of the
classical limit is accomplished via the on-shell leading-singularity method and
using massive spinor-helicity variables. The three-point amplitude for
arbitrary-spin massive particles minimally coupled to gravity is expressed in
an exponential form, and in the infinite-spin limit it matches the
stress-energy tensor of the linearized Kerr solution. A four-point
gravitational Compton amplitude is obtained from an extrapolated soft theorem,
equivalent to gluing two exponential three-point amplitudes, and becomes itself
an exponential operator. The construction uses these amplitudes to: 1) recover
the known tree-level scattering angle at all orders in spin, 2) match previous
computations of the one-loop scattering angle up to quadratic order in spin, 3)
lead to new one-loop results through quartic order in spin. These connections
map the computation of higher-multipole interactions into the study of deeper
orders in the soft expansion.